Wednesday, 30 April 2025

Thomas Cooke telescope and observatory for sale in Liverpool in 1885

 Pall Mall Gazette Friday 2nd January 1885

  

ASTRONOMICAL OBSERVATORY WITH  TELESCOPE AND APPOINTMENTS COMPLETE. 

To be SOLD, a bargain, on account of the owner's eyesight, an excellent Equatorial-mounted  TELESCOPE by Cooke, 4.5 inch diam.; Dawe's solar and numerous other eyepieces, micrometer, induction  coil and battery, automatic and star spectroscopes, spark condenser, clock by Cooke, barometer 7-10  diam., observing chair, complete sets of the memoirs and monthly notice's of the R.A.S., Astronomical Register and Observatory,  with indexes, and a number of other astronautical works, all in the best possible condition. The above presents a very rate opportunity  to astronomical students

 Address  "Telescope," care of Lee and Nightingale, Advertising Agents,  Liverpool.



                                                       www.theramblingastronomer.co.uk

Tuesday, 29 April 2025

T. Cooke &Sons telescope part of auction in London in 1882

 London Evening Standard Wednesday 3rd May 1882 

 

MESSRS. SOTHEBY, WILKINSON,& HODGE will SELL by AUCTION, at their House, No. 13, Wellington Street Strand  W.C. on Thursday May 25th the SILVER PLATE (above 1,000 ounces) and articles of Virtu, collected by the late John Fitchett Marsh esq, comprising plated ware, oriental, wedge wood and other china. Shakespeare relics some important bronzes, marble busts, marqueteric cabinets a  large and beautiful portable equatorial telescope by Cooke and Sons, 2 microscopes, one a very fine ‘binocular’ by Smith and Beck fire screens etc. 

John Fitchett Marsh Esq formerly of Fairfield House Warrington and late of Hardwick House Chepstow 

The sale of effects lasted for 9 days.


                                                        www.theramblingastronomer.co.uk

Monday, 28 April 2025

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE tonight and every Monday evening from 7.00 pm-9.00 pm on the award-winning Astronomy Show on Drystone Radio, probably the only regular astronomy show on any radio station in the country. 

I will take my weekly look at the night sky and look at all the latest news in astronomy. There will be the astronomical anniversaries this week plus the latest news from the astronomical societies in the north of England.

 


The Astronomy Show every Monday evening only on Drystone Radio live online at www.drystoneradio.com DAB radio in Bradford and East Lancashire, or 102 and 103.5 FM and can also be heard later on the Drystone Radio Podcast.

 

Second hand Cooke telescope for sale in Liverpool in 1875

 Liverpool Daily Post Thursday 5th August 1875 

Second hand astronomical telescope for sale by the late Mr Cooke of York- G S Wood (late Abraham & Co) Opticians 20 Lord Street Liverpool. 

In 1864 Abraham & Co had ordered a plain equatorial mounting on tripod for a 4.5 inch tube.


                                                        www.theramblingastronomer.co.uk

Sunday, 27 April 2025

The Sunderland Scientific and Industrial Exhibition in 1882 and a Cooke telescope

 Sunderland Daily Echo and Shipping Gazette Friday 17th February 1882

 The exhibition will be held at the Skating Rink Hudson Road and included Mr John G Allison of the Old Rectory Monkwearmouth, who exhibited a portable telescope which will be found worthy of our astronomical students. 

The object glass in 4 inches in diameter and 5 feet focal length withy polished brass tube and finder attached. It has 4 eyepieces powers from 80 to 300 and is fixed on a strong polished walnut tripod stand. 

I believe this the telescope purchased by John G Allison in 1866 from Thomas Cooke and Sons when Mr Allison was living at 12 Cumberland Row Newcastle.



                                                     www.theramblingastronomer.co.uk

 


Saturday, 26 April 2025

The Patrickhill Observatory in Glasgow with a Cooke telescope

John Dansken who was born in Glasgow in 1836 was by profession a surveyor and an enthusiastic amateur astronomer  who built an observatory at his home in Patrickhill, Glasgow which included a 5 inch telescope by Thomas Cooke of York, there was also a larger 13 inch reflector made by D Hunter of Lanark.

 A number of smaller instruments were also housed there including telescopes by Wray and Dollond. He also had one of the finest astronomical libraries in the West of Scotland. John Dansken died in 1905.


                                                       www.theramblingastronomer.co.uk

Friday, 25 April 2025

Ariel 1 the first British satellite was launched on April 26th1962

 On April 26th 1962 Ariel 1 the first British satellite was launched, it carried 6 experiments, Ariel 1 made the UK only the third country to have a satellite in space at that time. The others being the USA and the Soviet Union. 

Ariel 1 which was named after a Shakespearian character from the Tempest was launched by an American rocket. One of the missions of Ariel 1 was to measure solar radiation.  The UK did not have  the ability to launch a satellite at this time. 

Sadly its career was ended on July 9th 1962 when the Americans exploded their Starfish Prime atomic bomb in a high altitude test. The solar panels were destroyed and all contact with Ariel1 was lost.

Originally designed to re enter the atmosphere in 1963 it came down in 1976.


                                                       www.theramblingastronomer.co.uk


Wednesday, 23 April 2025

A little ramble through Auriga the Charioteer

 In wintertime Capella which is the brightest star in the constellation of Auriga the Charioteer is directly overhead. A striking constellation in the northern skies, Auriga lies above the horns of Taurus the Bull and forms the shape of a kite.

 Auriga is named after the son of Vulcan who invented the four-horse chariot. Another Greek legend associates Auriga with Myrtilus who was Hermes’s son and the charioteer of Oenomaus . The association of Auriga and Myrtilus is supported by depictions of the constellation, which rarely show a chariot. Myrtilus's chariot was destroyed in a race intended for suitors to win the heart of Oenomaus's daughter Hippodamia. Myrtilus earned his position in the sky when Hippodamia's successful suitor, Pelops, killed him, despite his complicity in helping Pelops win her hand. After his death, Myrtilus's father Hermes placed him in the sky.

In Greco Babylonian times the constellation was called Rukubi the Chariot. Arabic astronomers called the constellation Dhu al Inan the Rein Holder. If we look even further into the story we see even different ideas from ancient civilisations. Some Egyptians suggest that it represents Horus. In Chinese mythology, Auriga's stars were incorporated into several constellations, including the celestial emperors' chariots, made up of the modern constellation's brightest stars.


The brightest star in Auriga is Capella which is the 6th brightest star in the sky. Capella whose name means the Goat Star, which is the same name given to the star by the Sumerian astronomers. However Arabic astronomers called it Al Rakib the driver because it lies so far north it was prominent in the evening sky before other stars became visible and so apparently is watching over them. It has a magnitude of 0.1 and it’s a G class giant star slightly cooler than our Sun and is 43 light years distant.

In 1899 astronomers discovered that Capella was not a single star but a double star. But there's more going on with Capella as there is another component to this system, a pair of small red stars, meaning that where we see just one star there are actually 4!

In brightness it is virtually equal to Vega in the constellation of Lyra the Lyre but it is of a very different colour, its yellowish tinge contrast sharply with the steely blue of Vega. Both are circumpolar from Britain, they can be seen all year round, although they both will get very close to the horizon as seen from Britain. They lie on opposite sides of the north pole star and at roughly the same distance from it. This mean that when Capella is high up Vega is low down and vice versa. From Britain Capella is overhead during winter evenings while in summer it is Vega that occupies that position.

Slightly to the right and just below Capella is a little but quite distinct triangle of stars called the Haedi or the kids. They are referred to as the Kids because where the she goat goes the baby goats or  kids will always follow!! The top star in the triangle is epsilon, bottom left star is eta and the bottom right is zeta.

Epsilon was known to the Arab astronomers as Al Maaz the He Goat. To  Ulug Beg as Al Anz the meaning of the name appears to be unknown. Epsilon is a F class  supergiant white star its distance in not known with any great certainty, but it could be about 2,000 light years away. It normally it shines at around magnitude 3.0 but every 27 years it fades to magnitude 3.8 where it remains for between 640–730 days – about two years. Epsilon is eclipsed by an unseen and unknown very large companion star or cloud of dust.  The star’s last dimming was from 2009 to 2011.  The next should begin around 2038!

Zeta was known to the Arabic astronomers as Al Said al Thani or The Second Arm. Zeta is another eclipsing binary where the companion star cannot be seen with the naked eye and varies between magnitude 3.7-4.1 over a period of 972 days.  Zeta is a K class giant star lying 790 light years away.

The third component eta has no name. It lies 243 light years away. It is a B3 class star making it much hotter than the Sun, eta has a brightness of magnitude 3.2.

Beta or Menkalinan which means ‘Shoulder of the Charioteer’, is the second brightest star in Auriga and is found to the left of Capella with a magnitude of 2.0 the same brightness as the North Star. It is an A class star with a surface temperature of around 8,8,00 degrees much hotter than our Sun. It lies at a distance of 82 light years.

A line drawn down from beta will reach the star theta or Mahasin with means the ‘Wrist of the Charioteer’. Theta has a magnitude of 2.6 and is an A class star 166 light years away. 

From eta which is the top star of the Haedi or kids a line drawn down and past zeta will come across iota or Al Kab which means the ‘Shoulder of the Rein holder’ this is the same name as beta, a charioteer can be seen as the same as a reign holder. It is quite common for different names of stars to have the same meaning. Iota lies at a distance of 490 light years and has a magnitude of 2.7. It is a K class giant star  making it cooler than our Sun.

In 1930 for some reason the star that was originally classified as gamma Auriga whose name was also known as Al Kab which means the wrist of the reign holder was transferred to the constellation of Taurus the Bull and re labelled at beta Tauri. It makes no sense at all as it is the bottom of the kite shape which used to form Auriga. Again, this is a situation that in some star maps pre 1930 sometimes the star was sometimes placed in Auriga and other times put into Taurus.

There are some interesting variable stars in Auriga one is AE Auriga which normally shines at magnitude 6.0 which is the limit of naked eye visibility under the very best of sky conditions. However, it does vary irregularly. It is passing through the Flaming Star Nebula, this is a nebula that reflects light from nearby stars. This nebula is about 9 light years wide and it’s believed that AE Auriga has only recently entered the nebula.

There was a nova in Auriga in 1891 and is listed as T Auriga. When it was discovered, It had a magnitude of 5.0 on January 23, 1892, by Thomas David Anderson 1853-1932 who was a Scottish amateur astronomer It became visible to the naked eye by December 10, 1891, as shown on photographic plates examined after the nova's discovery. It then brightened from December 11 to December 20, when it reached a maximum magnitude of 4.4. T Auriga faded slowly in January and February 1892, then faded quickly during March and April, reaching a magnitude of 15 in late April, at which point it could only be seen with a fairly large telescope.

There are 3 messier objects in Auriga, they are all open clusters which are young groups of stars only a few million years old and contain only  a few dozen or few hundred stars each.

 M36 the Pinwheel Cluster which is an open cluster around 4,100 light years away. You cannot see it with the naked eye with a magnitude of 6.3 you would need a pair of binoculars to see it.

M37 is another open cluster at magnitude 6.2 although it is the brightest of the three open clusters in Auriga you would still need a pair of binoculars to find it.  It is 4,500 light years away.

M38 The Starfish Cluster is the faintest of the open clusters here at magnitude 7.4. It is around 4,200 light years away.

 


                                                    www.theramblingastronomer.co.uk

Tuesday, 22 April 2025

Alexander Herschel buys a Cooke telescope in 1867

 In 1867 Alexander Herschel purchased a small telescope from Thomas Cooke & Sons of York. It was a small telescope with an object glass of just 1.5 inches with a large field and short focus. The instrument was painted black. 

Alexander Stewart Herschel (1836-1907) was the son of John Herschel a polymath who spent time in South Africa cataloguing the southern sky. Alexander Herschel’s grandfather was William Herschel who in 1781 discovered the planet we now call Uranus.

 Alexander was less well known than his father or grandfather but he undertook pioneering work in meteor spectroscopy and worked in trying to identify comets as the sources of meteor showers.


                                                        www.theramblingastronomer.co.uk

Monday, 21 April 2025

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE tonight and every Monday evening from 7.00 pm-9.00 pm on the award-winning Astronomy Show on Drystone Radio, probably the only regular astronomy show on any radio station in the country. 

I will take my weekly look at the night sky and look at all the latest news in astronomy. There will be the astronomical anniversaries this week plus the latest news from the astronomical societies in the north of England.


The Astronomy Show every Monday evening only on Drystone Radio live online at www.drystoneradio.com DAB radio in Bradford and East Lancashire, or 102 and 103.5 FM and can also be heard later on the Drystone Radio Podcast.

Comet Swift 1892 observed from Sunderland with a Cooke telescope

 TW Backhouse of Sunderland using his 4.5 inch Thomas Cooke & Sons telescope reports on comet Swift 1892. He says that there appeared to be little notice of this comet. Backhouse said that he saw the comet on April 26th 1892 through a miniature spectroscope on his Cooke telescope. 

Although the best views of the comet so far were obtained on April 29th when although faint it was visible to the naked eye. The comet had a tail 11 degrees long. On April 30th the head of the comet was about 4th magnitude and was seen between mu and lambda Pegasus.



                                                        www.theramblingastronomer.co.uk

Sunday, 20 April 2025

Two Cooke telescopes in Brighton

 In 1857 Charles Howell (1783-1867) of Hove, Brighton purchased a 6.25 inch Thomas Cooke of York telescope, it was similar in design to the one that was exhibited at the Paris Exhibition in 1855. 

The telescope would be placed into an observatory, which I believe was built locally and not a Cooke observatory. Later after 1864 he also purchased a 7.5 inch Thomas Cooke & Sons telescope. It was this telescope that Mr Fry used to photograph the Moon with in 1865. This telescope was housed in a separate observatory and again this observatory appears to be locally made.

 He was also interested in double stars and planets, and because of his age he often let his many friends in the Brighton area use his telescopes.




 

Saturday, 19 April 2025

A small Cooke telescope for a Caledonian Railway worker

 John Robertson of Coupar Angus 1830-1920 owned a fine Thomas Cooke of York 3 inch refractor telescope. His interest in astronomy began in 1848 when he heard Dr Thomas Dick give a series of astronomical lectures. 

He spent many hours observing the sky, including sunspot observations and comets and meteors.  He was self educated and he had to fit all his observations of the sky around his work. He was employed by the Caledonian Railway. 

He sent many articles to newspapers including the Scotsman and some of the Dundee Daily newspapers. Among the astronomers he correspond with were Sir W.H. M. Christie, Richard A Proctor, Sir Robert Ball and Ralph Copeland. 

He was still using the 3 inch Cooke telescope as late as August 1917 to observe sunspots, with his advanced age his daughter had to help move and adjust the telescope.


                                                        www.theramblingastronomer.co.uk

Friday, 18 April 2025

Transit of Mercury seen in 1878 with a Cooke telescope from Peebleshire

 Robert Mathison of Innerleithen Peeblesshire observed the Transit of Mercury on May 6th 1878 using a Thomas Cooke of York 4.1 inch telescope. 

The transit was seen from the ‘observatory’ no trace of the planet could be seen outside the disk of the Sun. A small group of sunspots were seen on the Sun close to the planet at 4.40 pm. 

One point that caught the attention of Mathison was that a bright white point of light which he followed until 5.30 pm when the Sun was covered by clouds. Other observers at this location confirmed the sighting of the bright white spot.


                                                        www.theramblingastronomer.co.uk

Thursday, 17 April 2025

A little ramble through Aries the Ram

 A constellation that dates to ancient times, in legend Aries represented the Ram whose golden fleece was sought by Jason and the Argonauts. If you watch the film Jason and the Argonauts, you will get an idea of the story.

The Euphratean astronomers knew it as Gam, the scimitar the curved blade being formed from stars in Pisces and the last three bright stars in Aries. This was the weapon protecting the kingdom against the seven evil spirits or Tempest Powers. Some people think the figure was designed to represent the Egyptian King of gods shown at Thebes with ram’s horns and known by a variety of names including Amon, Hammon and Amen. The Arab astronomer Ulugh Beg 1394-1449 called the constellation Al Kabas al Alif or the Tame Lamb.

Despite not being a very bright constellation, it has assumed great importance in astronomy, because around 2,000 years ago it contained the point where the Sun passed from south to north across the celestial equator each year. This point, the vernal equinox marked the start of spring in the northern hemisphere.

This point is known as the first point of Aries. However, because of the slight wobble of the Earth which is called precession this point has now moved into the neighbouring constellation of Pisces. Having said that we still call it the First Point of Aries.


The brightest star, alpha is called Hamal which means ‘The Head of the Sheep’, it shines at magnitude 2.0 the same brightness as the North Star. Hamal lies 66 light years away and is a K class giant with a surface temperature of 4,200’C compared to 5,800’C of the Sun. The astronomers Ptolemy and Ulugh Beg both describe the horn of the ram as being over the head, Hipparchos in his star map who described it as being on the muzzle. It was the last of the great telescope astronomer Tycho who placed the horn back on the head of the ram as we see it depicted today.

The next brightest star is beta which is called Sheratan meaning ‘The Sign’ and is 60 light years away it has a magnitude of 2.7. Sheratan is an A class star with a temperature of 8,700’C much hotter than the Sun.

A line drawn from Hamal and to the left and upwards slightly will reach the third brightest star in Aries. This is 41 Arietis. I know I have said that the brightest 24 stars of each constellation have a Greek letter allocated to them. The first Astronomer Royal John Flamsteed (1646-1719) undertook a survey of the night sky and gave every naked eye star in a constellation a number, evens stars which have a Greek letter. Sometimes this system is totally disregarded.

41 Aries has a magnitude of 3.6 and is a B class star hotter than our Sun and is 166 light years distant. The star does not have a Greek letter because it was originally part of a now defunct small constellation called Musca Borealis the Northern Fly.

Just below beta you will find gamma or Mesarthim the meaning is unknown; its magnitude is 3.9 and is 164 light years away Mesarthim is a B class star much hotter than the Sun.  The star used to be called ‘The First Star of Aries’ as it was the closest visible star to the vernal equinox .

There is a meteor shower the Arietids which are active between May 22nd and July which peaks on June 7th. Sadly, it is invisible to the naked eye because it is a daytime meteor shower. This meteor shower and there are many daytime showers are studied by astronomers using radar or radio telescopes.



                                                      www.theramblingastronomer.co.uk

 

 

 

 

Wednesday, 16 April 2025

A Thomas Cooke telescope in Whitby

 There is a 5 inch Thomas Cooke and Sons telescope located in an observatory in the grounds of Whitby Community College which today is Whitby School. 

The telescope dates from about 1880/1890 and was used between 1912 until 1932 by Mr John  Bruce and the observatory is typical of a late 19th early 20th century design. Today the observatory is known as the Bruce Observatory. 

The observatory appeared to be in use until the 1960s by the school physics department. I am not sure when it started to be less used but when I visited the observatory in the mid 1990s both the telescope and observatory needed some attention.

 That seems to have been undertaken as the telescope is often used by the Whitby& District Astronomical Society who organise astronomical events there.   


                                                         www.theramblingastronomer.co.uk

Tuesday, 15 April 2025

The 1868 Transit of Mercury seen from Liverpool with a Cooke telescope

George Williams using a 4.25 inch Cooke & Sons telescope observed the transit of Mercury on November 5th 1868 from 2, Devonshire Road, Prince’s Park, Liverpool. 

Williams observed no apparent elongation or pear shape, or black drop at the egress of the planet; but the boiling of the limb, which was considerable, may account for the absence of these appearances.


                                                    www.theramblingastronomer.co.uk

 

 

Monday, 14 April 2025

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE tonight and every Monday evening from 7.00 pm-9.00 pm on the award-winning Astronomy Show on Drystone Radio, probably the only regular astronomy show on any radio station in the country.

I will take my weekly look at the night sky and look at all the latest news in astronomy. There will be the astronomical anniversaries this week plus the latest news from the astronomical societies in the north of England.

 The Astronomy Show every Monday evening only on Drystone Radio live online at www.drystoneradio.com DAB radio in Bradford and East Lancashire, or 102 and 103.5 FM and can also be heard later on the Drystone Radio Podcast.

 

Martian Moons seen with a Cooke telescope in 1881 from Sunderland

On December 22nd 1881 John Watson of Sunderland (more accurately Seaham Harbour, which is about 5 miles south of Sunderland) reported seeing two small points of light near Mars using a Thomas Cooke & Sons 12inch refractor. The positions of the moons were determined  by using the ephemeris of Mars is indicated where the two satellite should be. 

I have little more information regarding either this 12 inch telescope or observations made by it. Although it is mentioned in G F Chambers Handbook of Descriptive and Practical Astronomy vol. 2 Oxford 1890 page 297. 

Watson had an 8 inch Wray telescope mounted on a metal pillar supplied by Thomas Cooke which he offered for sale in 1880 presumably to make room for the 12 inch Cooke.


                                                         www.theramblingastronomer.co.uk

Sunday, 13 April 2025

A little ramble through Ara the Altar

 Ara the Altar lies in a dense part of the Milky Way immediately south of the hook of stars that make up the tail of Scorpius the Scorpion. This means that it is a summer constellation. It is invisible from Britain but has been known since ancient times, remember that many of these constellations were created in Greece or by peoples living near the Mediterranean. This means that from these areas this constellation will be seen much higher in the sky.

Although a relatively minor group with no named stars in Greek mythology, Ara represented the altar used by Zeus and other Greek gods to swear a vow of allegiance before they went to war against Cronus and the Titans. According to legends, it is believed the Cyclops originally built the altar as a place to sacrifice to the Olympian gods. It was also upon this altar that Centaurus the centaur sacrificed Lupus the wolf.

In Arabia it was Al Mijarah or a censer which means it had no shape before the introduction of Greek mythology. However in Chinese astronomy the stars that form Ara are part of the Azure dragon of the East, this is one of the dragon gods .


Ara has a fairly distinctive shape, its brightest stars are:-

Alpha , the second brightest star can be found below the bright star theta in the tail of the  Scorpion. Alpha has a magnitude of 2.9 and is 270 light years away. It is a B class star with a surface temperature of around 17, 700 degrees compared to 5,800 degrees  of our Sun.

A line drawn down from alpha leads to beta, the brightest star in Ara which has a magnitude of 2.8 and is 650 light years distant. It is a K class super giant star with a surface temperature of 3,800 degrees indicating it is cooler than our Sun.

Just underneath beta is gamma, located 1110 light-years from Earth, and is a B1 class supergiant with a whopping surface temperature of 21,200 degrees with a magnitude of 3.3.

 Continuing a line further down we reach delta with a magnitude of 3.6 it’s a B 8 class star indicating that it is much hotter than the Sun. Delta lies 198 light-years from Earth.

A line drawn from beta to the right will lead you to zeta the third brightest star in Ara with a magnitude of 3.1. Zeta is a K3 giant star with a surface temperature cooler than the Sun, it lies 490 light years away. As zeta is the 5th letter of the Greek alphabet it should be the 5th brightest star here. It isn’t which again shows that the Bayer system of using Greek letters in constellations does not always work.

From zeta a line drawn down and slightly to the right leads to eta which is about 299 light years away, eta is somewhat fainter than other stars in Ara  with a magnitude of 3.8. Another K class star.

Since Ara contains part of the Milky Way to the south of Scorpius, it therefore has rich in clusters of stars. There are no messier objects in Ara this might be because the constellation was too far south for him to easily observe it.

Ara gives us the chance to view the two types of clusters we see in the sky both are just visible to the naked eye if the sky conditions are very good. Open Clusters are groups of very young stars which are loosely held together by gravity and will over time drift apart over a period of several million years. Globular Clusters on the other hand are formed from very old stars.

Both clusters have NGC numbers which stand for the New General Catalogue (NGC) which was produced in 1888 and was an addition to the General Catalogue and Nebulae and Clusters that had been produced in the first half of the 19th century by William Herschel who had discovered the planet Uranus in 1781 and his sister Caroline and William’s son John Herschel.

NGC 6193 is open cluster which can just be seen with the naked eye, although binoculars will make it more easily visible. There are 27 stars, it’s about 3 million years old and is about 3,800 light years away.  It was discovered by the Scottish astronomer James Dunlop 1793-1848 in 1826 while observing in Australia. Under the very beat of conditions, it can be just glimpsed with the naked eye but can be seen much easier with binoculars.

NGC 6397, is a globular cluster and is located about 7,200 light-years from Earth, making it one of the two nearest globular clusters to Earth  The cluster contains around 400,000 stars, and like NGC 6193 can be seen with the naked eye under good observing conditions but can easily been through binoculars. It was discovered by the French astronomer Nicolas Louis de Lacaille 1713-1762  in 1752 while observing from South Africa.


                                                     www.theramblingastronomer.co.uk


Saturday, 12 April 2025

Photos of Orion taken with a Cooke telescope from Newcastle in 1890

In 1890 Lawrence Richardson of Newcastle on Tyne using a 4.5 inch Thomas Cooke & Sons telescope undertook some research into astronomical photography using his telescope which was an achromatic.  He was not that hopeful of getting really sharp images, the Cooke & Sons photo visual telescope would not be available until he mid 1890s. 

Richardson found that he could take a photograph of Orion which would show hundreds of stars and which would take around about an hour. He went on to say that he thought that astrophotography was a very good field for amateur astronomers to work in and obtain good results.


                                                      www.theramblingastronomer.co.uk

Friday, 11 April 2025

Even a Thomas Cooke telescope cannot see through trees.

 Mt T H Waller of York in 1865 and using a 4.75 inch Cooke telescope was trying to observe the satellites of Jupiter when unfortunately, the planet was obscured by some trees, and he was unable to see the immersion of the second satellite or the transit of the third. Fortunately, by the time that the fourth satellite was passing in front of Jupiter it had cleared the trees. 

Mr Waller was also a very keen double star observer he would often use the double star catalogue of Mr Brothers of Manchester and the Bedford Catalogue.


                                                         www.theramblingastronomer.co.uk

 

Thursday, 10 April 2025

April Full Egg and Micro Moon

On the night of the 12th/13th April the Moon will be full this is the Egg Moon. 

Many press agencies are now using the American names for the full moons. It is often referred to as the Pink Moon because of the pink phlox flowers that can be seen in America at this time of year. These American names are only a couple of hundred years old. I prefer to use the old monastic names of the full moons which go back over 1,200 years.

The full moon in April is the Egg Moon, this has nothing at all to do with Easter Eggs. It is due to the fact that at this time of year the nights are getting shorter the length of daylight  increases so the ducks, geese and hens that the monks own start to lay more eggs. Hence the Egg Moon.

April also sees the closest Micromoon of the year. Many people will have heard of the Supermoon when the moon looks larger tin the sky than normal, this is because the moon is a little closer to us than normal. There are however times of the year when the moon is a little further away and this makes the moon look smaller.

So if you see the Full Egg Moon this weekend you are also looking at the furthest  full moon  of the year.


                                                       www.theramblingastronomer.co.uk

Sunspot group seen from Leeds in 1930 with a Cooke telescope

 In October 1930 Mr Tetley of Headingley, Leeds used his 4 inch Thomas Cooke & Sons telescope to observe the Sun. He took some photographs of the great sun spot group of October that year. In particular on October 10th the photographs very clearly showed the changes which took place in the groups which crossed the central meridian

 


                                                      www.theramblingastronomer.co.uk

Wednesday, 9 April 2025

A little ramble through Aquila the Eagle

 Aquila the Eagle is supposed to represent a bird figured on a Euphratean uranographic or star map from about 1200 BCE. It is one of the original 48 constellations still used today. The constellation as often associated with Zeus and often carried his thunderbolts.

Most ancient civilisations seem to associate Aquila as either an eagle or bird of some kind. Some mythologies associate the bird as a vulture rather than an eagle, the Romans and the Mongols did. Old stories talk about the eagle carrying the shepherd boy Ganymede to  Zeus.

Aquila is a summer constellation and its brightest star Altair which means flying eagle is part of a very familiar group of stars in the summer sky known as the Summer Triangle. It is the closest of those three stars being only 17 lightyears away, while Vega in the constellation of Lyra the Lyre is 25 light years away and Deneb in Cygnus the swan a massive 2200 light years away are the other two stars in the triangle.


Altair is magnitude zero star and is an A class star making it hotter than our Sun. It is a star that rotates very quickly meaning that it is not spherical in shape because it is flattened at the poles due its high rate of rotation.

Altair and the two stars that are either side of it beta and gamma were known as the family of Aquila while the Chinese knew this little group as Ho Koo a River Drum.

For any fans of the film Ben Hur one of the horses in the great chariot race at Antioch one of them was Aquila.

Gamma or Tarazed which means the balance is the next brightest star in Aquila, it is the brighter of the two stars that flank Altair. The star is 395 light years away and is a K class giant star. It is cooler than the Sun with a surface temperature of around 4,000 degrees. It’s a young star only around 270 million year old and although it is  more massive than the Sun it will not destroy itself in a supernova explosion it will simply expel its outer layers of gas into space, become a planetary nebula and then ultimately a small white dwarf star as it reaches the end of its life.

Zeta also known by its Arabic name as Deneb el Okab which means the tail of the eagle has a brightness of magnitude of 3 and is a double star and is around 83 light years away . Its an A class star meaning its hotter than our Sun.

Delta Aquilae is slightly fainter than zeta ay mag 3.3  it’s  an F class star slightly hotter than the Sun, and lies about 50ly .

If you have wondered what has happened to Beta Aquila well it’s here its name is   Alshain which like gamma also means balance is the other star flanking Altair. It should according to the Bayer system using the letters of the Greek alphabet be the second brightest star in Aquila in fact it comes in as the 5th. I have  no idea why.  Alshain is a G type star slightly cooler than the Sun and is located 45 light-years from Earth. To the eye it is a single star however it is in fact a triple star system.

Eta Aquilae is a variable star discovered by Edward Piggot on September 10th 1784 in York, this was a  night to remember in York , as the deaf astronomer John Goodricke discovered the variability of the star Beta Lyra. I christened Goodricke and Pigoiott as the Fathers of Variable Star Astronomy for all the work they undertook in that field of astronomy. Eta is a cepheid type variable the first Cepheid was of course discovered by Goodricke from York!!

A cepheid variable star is a distance marker in the galaxy. Cepheid variable are a class  of variable stars whose periods of variation are closely related to their luminosity and that are therefore useful in measuring interstellar and intergalactic distances. Most are spectral type F (moderately hot) at maximum luminosity and type G (cooler, Sun-like) at minimum.  In 1912 Miss Henrietta Leavitt of Harvard Observatory discovered the period-luminosity relationship of the Cepheids in the Large Magellanic Cloud and the Small Magellanic Cloud. These are two satellites galaxies to our own Milky Way Galaxy. This work helped show that these nebulous patches in the sky were not in our galaxy but were galaxies in their own right. Today we know they are around 160-170,000ly.

A bright nova appears over the Western Front during World War 1. Nova Aquilae 1918 was, first seen June 8th, 1918. First seen by the Polish medical professor and amateur astronomer Zygmunt Laskowski it was confirmed   Britain by the amateur astronomer Grace Cook.  Nova Aquila was the brightest novae seen during the last 300 years reaching a mag of -0.5. Because the milky way passes through Aquila 9 nova have been seen in the last 120 years, most have been faint but you never know a bright one might be coming in the near future is it is always worthwhile looking at this part of the sky.

There are no Messier objects in Aquila which is surprising, since the constellation lies along the northern Milky Way between the rich star clouds of Cygnus and the galactic opulence of Sagittarius.

 Perhaps the finest open cluster  in Aquila is NGC 6709. Open clusters are groups of young stars. This cluster is believed to be around 300 million years old. It’s a sprawling irregular group of stars which, to some stargazers, looks like a sparkling unicorn. NGC 6709 is about 3,900 light years away and spans about 17 light years. 

The constellation is also home to NGC 6751, a planetary nebula. that is also known as the Glowing Eye. The nebula is estimated to be around 0.8 light-years in diameter and is estimated to be roughly 6,500 light-years away from Earth. It was formed when a star collapsed and threw off its outer layer of gas several thousand years ago.

The word "nebula" is Latin for mist or cloud and the term "planetary nebula" is a misnomer that originated in the 1780s with astronomer William Herschel because when viewed through his telescope, these objects resemble the rounded shapes of planets. Herschel's name for these objects was popularly adopted and has not been changed.

They are a relatively short-lived phenomenon, lasting a few tens of thousands of years, compared to a typical stellar lifetime of several billion years. 

And finally NASA's Pioneer 11 space probe, which flew by Jupiter and Saturn in the 1970s, is expected to pass near the star Lambda  Aquila in about 4 million years.


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Tuesday, 8 April 2025

Spot on Saturn seen from Sunderland in 1890 with a Cooke telescope

 Dr J Haswell, Grange Terrace, Sunderland  observed the spot on Saturn that had been seen by Dr Terby in March 1890. He saw the spot on several  nights in March , and he described it as being very obvious on March 30th, though not so noticeable as it had been last spring. 

Haswell used a 4.25 inch Thomas Cooke & Sons telescope which was of short focal length.


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Monday, 7 April 2025

The Astronomy Show on Drystone Radio

 Join me, Martin Lunn MBE tonight and every Monday evening from 7.00 pm-9.00 pm on the award-winning Astronomy Show on Drystone Radio, probably the only regular astronomy show on any radio station in the country. 

I will take my weekly look at the night sky and look at all the latest news in astronomy. There will be the astronomical anniversaries this week plus the latest news from the astronomical societies in the north of England.


The Astronomy Show every Monday evening only on Drystone Radio live online at www.drystoneradio.com DAB radio in Bradford and East Lancashire, or 102 and 103.5 FM and can also be heard later on the Drystone Radio Podcast.

 

Sunspots observed with a Cooke telescope in Somerset in 1929

 Mr R. L. Robinson, Minehead, Somerset using a Thomas Cooke and Sons 6 inch telescope made a series of drawings of sunspots large and small in October, November and December 1929. These spots were of considerable interest because they rapidly changed in appearance on a daily scale. 

In many cases details of structure were obtained using a Dawes eyepiece, by which a great deal of the surrounding photosphere can be shut off or even a large part of a spot can be isolated. This is often a great advantage, especially in observing the changes of detail in a bridge or projection.


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Sunday, 6 April 2025

A little ramble through Aquarius the Water Bearer

 Aquarius is one of the most ancient of constellations. The Babylonians saw this area of sky as a man pouring water from a jar and it is still represented this way today. Aquarius is one of the zodiacal constellations and according to the Greeks it is linked to Ganymede, cup bearer to the Olympic gods.

It’s in the Zodiac a belt of stars made up of 12 constellations that stretch around the sky, actually there are 13 constellations in the Zodiac, no one ever talks about Ophiuchus. The zodiac is where the Sun, Moon and planets will always be found in the sky. Many people get confused with astronomy and astrology, astronomy is the science of the stars while astrology is the pseudo-science that tries to link people’s characteristics with the positions of the planets against the starry background.

The Arab astronomer Al Biruni saw it as Amphora a two handled wine jar. The Egyptians referred to the constellation as Monius or water. While in China with Capricorn, Pisces and a part of Sagittarius it was seen as a serpent or turtle. The Anglo Saxons called it se Waeter-gyt the water pourer.

Although Aquarius which can be seen in the autumn is the 10th largest constellation is not a particularly bright one. It can be found below the square of Pegasus. The most prominent part of the constellation is the Y shaped figure of 4 stars representing the water jar itself centred on the star zeta. Together with gamma, eta and pi this little area is often called the ‘Water Jar’. With it being low in the sky any mist or moonlight means that not even the brightest stars can be seen with the naked eye.


The brightest star is not alpha but beta whose name is Sadalsuud which means ‘luck of lucks’ is of mag 2.8 and is about 540 light years away. It is a G class supergiant with a temperature of 5,400`C slightly cooler than the sun.

The second brightest star is alpha at mag 2.9 is another  G class supergiant star, again slightly  cooler than the Sun it has a proper name which is sadalmelik which means ‘luck of the king’. Alpha is about 520 light years away. It has a surface temperature of around 4,900`C.

Delta or Skat which means ‘leg or shin’ is the third brightest star at magnitude 3.3 and about 113 light years away. It is an A class star with a surface temperature of about 8, 700`C much hotter than the Sun.

The following stars make up the water jar

Gamma or Sadachbia, its name means ‘luck of the homes’ (tents).The star has a magnitude of  3.8 and is 164 light years distant. It is an A class star with a surface temperature of about 10,200`C, our Sun is about 5,800’C

Zeta which is slightly above and to the left of gamma is an unnamed and  is a binary star, which means there are two stars here, however without a small telescope you would not be able to see the two stars. Zeta is located at the centre of the water jar asterism. The two stars are yellow white type stars one is a F3 star at magnitude 4.2 the other a F6 giant at magnitude 4.5 . Both are hotter than the Sun . The pair are 92 light years away and when we put the brightness of the two stars together they appear in the sky as a single star to the naked eye as a star of magnitude 3.6.

To the left of zeta is eta is a star of magnitude 4.0 and is 168 light years away, It is a B class star with a surface temperature of 11,000 degrees ‘ C twice the temperature of the Sun.

Just to the right of zeta is pi the faintest of the water jar group of stars at magnitude 4.6, it is a B class  giant star with a whopping large temperature of 26,700’ C. Pi is 780 light years away.

One other star I feel I need to mention is :-

TRAPPIST -1 which stands for Transiting Planets and Planetesimals Small Telescope. A solar system with 7 Earth size planets. They all are between the size of Mars and Earth. The system lies around 40 light years away.  It is too faint to be seen with the naked eye.

As the title of the project indicates astronomer are searching for planets transiting or passing in front of the star they orbit. TRAPPIST -1 was discovered back in 2016.

The star in question here is a small red dwarf star. It is much smaller than our Sun. Astronomers want to know if any of the planets can support life. One big problem with red dwarf stars is that they produce very powerful flares which may make it very difficult if not impossible for life to exist on any plants orbiting a red dwarf star.

The idea of looking for a slight change in brightness of a star when something passes in front of it is not new. The idea was first put forward by the deaf astronomer John Goodricke in York in 1782. Collaborating with his colleague Edward Pigott together they observed a star in the constellation of Perseus. The star called ALGOL t marks the eye of the medusa. The star names are Arabic and Algol means the ‘Winking Demon’. We know today that Algol is a double star system and the stars are orbiting and eclipsing each other causing the brightness of the star to change. With the star names being Arabic I wonder if the Arab astronomers also realised that this star changed in brightness. If they did no records have survived. The light changes on Algol are much more than on TRAPPIST-1.

In the 18th century the French astronomer was looking for comets. He found around a dozen or so, non were particularly import, however he kept coming across a large number of fuzzy looking objects similar to comets. These caused him a lot of problems so he drew up a list on non-comet objects to avoid becoming confused with these objects. It is strange to report today that his comets are nearly forgotten to history but that his list of non-comet objects The Messier List of 110 objects is still used by astronomers today.

There are two Messier objects: -

 Messier 2

A globular cluster discovered by the Italian astronomer Maraldi on September 11th 1746, who believed it to be a nebulous star.  Globular clusters are densely packed collections of ancient stars. Roughly spherical in shape, they contain hundreds of thousands, and sometimes millions of stars.

Charles Messier rediscovered the cluster exactly 14 years later on September 11th 1760. It was only in 1783 that William Herschel who 2 years earlier had discovered the planet Uranus was able to see through a larger telescope and realise that M2 was made up of numerous stars.

M2 has a diameter of about 175 light years and contains about 150,000 stars, it is one of the most compact globular clusters, and most of the brightest stars are red and yellow giant stars. M2 appears to be about 13 billion years old that is about 3 times the age of the Earth and Sun. M2 is about 33,000 light years away.

M2 is  north of Beta Aquarii,  M2 has a magnitude of 6.5 which means that it is  below naked eye visibility but can easily been seen with a pair of binoculars. In binoculars it will appear as a large, fuzzy ball with little or no resolution. It is possible to just see some stars around the edge using a 6 inch telescope, a larger telescope above 10 inch will resolve into stars.

In the 1830s, John Herschel (son of William who discovered the planet Uranus in 1781)  saw it as “It is like a heap of fine sand!” which is perhaps as apt a description as can be rendered. Through a large telescope, the globular cluster does resemble a glittering mass of sparkling granules.

Messier 72 

M72 is east of the 3.8 mag star epsilon Aquarius, this is the faintest globular cluster in the Messier list.

At mag 9.2 this globular is easy to miss, M72 actually spreads across 98 light years and like M71 is classified as a good open globular, and  is 56,400 light years away.

It can just be glimpsed in larger binoculars but require a reasonable size telescope to see it well. The cluster is racing towards us at about 160 miles per second so maybe many 1000s of years from now owners of small telescopes will be able to see it better.

Messier first observed M72 in 1780 who said its light was faint

 

 

M73

This was one that fooled Messier in that it is not a star cluster of galaxy but just a close group of stars. A trio of 10th mag stars in a poor field is in Aquarius is how Admiral Smyth described this most unremarkable Messier object in his Cycle of Celestial Objects  published in the 19th century .

This group of stars is situated close to M72  and  is actually a grouping of 4 stars with no apparent connection, except that they lie in the same line of sight. Asterisms like this can be seen in any part of the sky. Messier just got fooled by it.

The optics of Messier’s telescope were not as good as modern optics and this is why the group probably looked fuzzy to him.  This could have been combined with poor atmospheric conditions when he observed them.

Messier first observed M73 in 1780 and described it as a cluster of 3 or 4 faint stars which at first glance resembles a nebula, and which does contain some nebulosity.

Although the stars appear to be close together in space in fact they are not. The stars are all at different distances to the Earth. The stars appear as an object of magnitude 9. They cannot be seen with the naked eye and a reasonably large telescope would b needed to see them.

There are two other nebulous objects to mention on Aquarius , the first is NGC 7009 the Saturn Nebula so named because it looks the planet Saturn. The letters NGC stand for the New General Catalogue that was introduced in 1888, even today we still use the term NGC. It is  a planetary nebula this is a star in the process of throwing all of its gas away into space before it becomes a white dwarf star. This is the ultimate fate for our Sun in a few billion years’ time.

It was discovered by William Herschel in 1783 he thought it looked a little like a planet hence the name planetary nebula. This nebula is around 5,200 light years away.

The name  Saturn nebula was given to the object by Lord Rosse from his observatory at Bir Castle in Ireland using what at the time was the largest telescope in the world. The telescope had a mirror 72 inches wide was built in 1845.

Here is another planetary nebula in Aquarius this is NGC 7293 the Helix Nebula which at 655 light years distance is the closest planetary nebula to us.

Meteor showers

There are two meteor showers associated with Aquarius. Meteors or shooting stars as many people like to call them are connected to comets. They have nothing at all to do with stars but are grains of dust that burn up as they enter the Earth’s atmosphere. A comet is a large dirty snowball travelling around the Sun, it leaves a trail of dust behind it and if the Earth happens to pass through one of these dust streams we see lots of meteors or a meteor shower. There are several meteor showers during the  year.

The eta Aquarids meteor shower occurs during early May with the maximum number of meteors seen around the 5th  May when around 40 meteors per hour can be seen. The meteor shower is so named because all the meteor in the sky seem to start their path across the sky from the star eta Aquarius. The comet connected with this meteor stream is none other than Halley’s Comet. There are two meteor showers connected with Halley’s comet, the other is in October and is called the Orionids.

The second meter shower is the delta Aquarids which peaks around abut July 30th when around 20 meteors per hour can be seen. This meteor shower is connected with comet Macholtz .


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Saturday, 5 April 2025

Asteroid Circe discovered 170 years ago on April 6th 1855

On April 6th 1855 the asteroid Circe was discovered by J Chacornae at Paris. Circe is named after the enchantress daughter of the Sun, celebrated fore he knowledge of magic and venomous herbs. Circe changed the companions of Odysseus into pigs. She had no influence on Odysseus because Hermes protected him. Odysseus lived a year with Circe, his friends were transformed into men.

Asteroid number 34 Circe  it is around 113 km across and orbits the Sun once every 4.4 years.


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Friday, 4 April 2025

Spectroscopic changes seen in 1906 in gamma Cassiopeia with a Cooke telesscope

 Stanley E Percival, Merriott Vicarage, Somerset observing with a 3.75 inch Thomas Cooke and Sons telescope reported that the bright hydrogen line C has been very bright recently in Gamma Cassiopeia. 

He reported on May 2nd 1906 that he failed to see the C line, while on May 4th he saw it quite distinctly. On May 18th although the sky was clear and the spectrum steady he barely glimpsed it. 

He notes that in Miss Clerke’s ‘Problems in Astrophysics’ page 248 that it has previously behaved in a capricious way, and if my small Cooke telescope is to be trusted it looks like it is doing so again.

 Spectroscopic changes appear to have started around 1927 so this could be a much earlier report than is generally accepted. The spectroscopic variations did seem to occur some years before the light changes were detected.

Today gamma Cassiopeia is the prototype of a class of eruptive variable stars, theses gamma Cassiopeia stars show irregular light variations of around one magnitude which can last for weeks or decades. Normally magnitude 2.2 gamma has been seen as faint as magnitude 3.0 and as bright as magnitude 1.6



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Thursday, 3 April 2025

A little ramble through Apus the Bird of Paradise

 Stars in the southern hemisphere were of course unknown to European astronomers because no one had travelled there before the 1400s. This is why most of the constellations in this part of the sky are referred to as modern constellations.

One example is Apus the Bird of Paradise which unfortunately like many of these modern constellations contains few if any bright stars. Johann Bayer called the constellation Apus Indica the Indian Bird. That title has been dropped today and it is just referred to as Apus.

Apus is what is called a circumpolar southern hemisphere constellation, this means that from countries like Australia and New Zealand it can be seen all year around. This is much like the familiar group of stars we call the Plough which can be seen all year from countries such as Britain and is called a northern circumpolar constellation.

This constellation is best seen in July which of course in the southern hemisphere is during the winter.

Apus the bird of paradise was introduced to the sky in the 1590s by the Dutch astronomer and cartographer Petrus Plancius from the observations of Dutch navigators Pieter Keyser and Frederick Houtman, when they voyaged to the southern hemisphere and visited countries such as Indonesia or what at that time was known as the Dutch East Indies.

Plancius had produced in 1589 a celestial globe using what information was available regarding the southern stars. These included constellations such as Crux the Southern Cross and Triangulum Australe the Southern Triangle as well as the Magellanic Clouds which were called Nubecula Major and Minor. These were reported by the Portuguese explorer Ferdinand Magellan c 1480-1521 as he journeyed around the world. These we know today are nearby Large and Small Magellanic Clouds which are nearby galaxies to our own Milky Way Galaxy.

Plancius knew that the Dutch navigators Pieter Keyser and Frederick Houtman would be travelling to the southern hemisphere so he met them and trained them to draw and note features in the sky so he could replicate them on a new star globe he was producing. With the knowledge that Keyser and Houtman provided Plancius in either 1597 or early 1598 produced a new celestial globe with an additional 12 constellations. None of these can be seen from Britain and they describe mostly animals and subjects that travellers of the day had seen as they explored the southern hemisphere.

The name of the constellation is derived from the Greek word apous, which means “footless.” (Birds of paradise were at one point in history believed to lack feet). The Greater Bird of Paradise known in India had a magnificent white, yellow and red plumage but unsightly legs, which were cut off by the natives desiring to offer the white man only the attractive part of the bird. There are no myths associated with the constellation.

In China the constellation was referred to as E Cho the Curious Sparrow or the Little Wonder Bird.


Apus is located near the south pole star, there are no bright stars in Apus, the brightest are alpha at magnitude 3.8 and is around 430 light years away. The sky must be clear and dark to see this star.  It is a K class giant star with a surface temperature of around 4,000 degrees it is cooler than the Sun.

Apus is an example of a constellation where using Johann Bayer’s Greek alphabet sequence does not work. This is because the second brightest star is gamma with a magnitude of 3.9 compared to the brightness of beta which is magnitude 4.2.

Although the Milky Way flows through Apus there are no bright clusters of stars to be seen. The brightest is NGC 6101 a globular cluster lying around 50,000 light years away. However, at magnitude 9.2 a telescope would be needed to see it.


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